Indeterministic Quantum Gravity IV. The Cosmic-length Universe and the Problem of the Missing Dark Matter
| dc.creator | Mashkevich, Vladimir S. | |
| dc.date | 1996-09-13 | |
| dc.date.accessioned | 2026-07-07T03:31:17Z | |
| dc.date.available | 2026-07-07T03:31:17Z | |
| dc.description | This paper is a sequel of the series of papers [gr-qc/9409010, gr-qc/9505034, gr-qc/9603022], being an immediate continuation and development of the latter of them. In the Friedmann universe, the equation $Ω_0=2q_0$ holds ($Ω$ is density parameter, $q$ is deceleration parameter, and subscript 0 indicates present-day values), which gives rise to the problem of the missing matter as observational data give $Ω_0<2q_0$. In the cosmic-length universe, $Ω_0=2q_0- L/R_0^3H_0^2$ ($R_0$ is the radius of the universe, $H_0$ is Hubble constant), which lifts the problem. The cosmic length, $L=const \approx 1/H_0$, is the infimum of the set of maximal radii of a closed universe. | |
| dc.description | 7 pages, LATEX 2.09 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9609035 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9609035 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35807 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.title | Indeterministic Quantum Gravity IV. The Cosmic-length Universe and the Problem of the Missing Dark Matter | |
| dc.type | text |